Neutrino Detectors Gary Barker (University of Warwick) PPAP, Uni. Birmingham , 18-09-12 Requirements of the detectors To have sensitivity to mass hierarchy and dCP.
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Neutrino Detectors Gary Barker (University of Warwick) PPAP, Uni. Birmingham , 18-09-12 1 Requirements of the detectors To have sensitivity to mass hierarchy and dCP in a single experiment will require: Target mass at least as big as T2K/SuperK and Nova To record neutrino interactions over a spread of energies (Wide Band Beam) Excellent reconstruction of kinematics (esp. En) Clean ne CC reconstruction (i.e. small nm CC and NC backgrounds) Ideally with charge reconstruction ability: Essential for a Neutrino factory beam to discriminate nm/anti- nm (Golden Channel) Unfolding the nm/anti- nm components of a conventional beam For a Particle Astrophysics/nucleon decay/geo-neutrino programme: Low threshold physics (< few tens MeV ): core collapse SNe, diffuse SNe remnants, thermonuclear solar neutrinos, geoneutrinos... 2 Main Technology Choices Iron/scintillator sandwich tracking calorimeter MINOS Liquid argon Liquid scintillator BOREXINO SUPERKAMIOKANDE Water Cherenkov 3 Pros and Cons Iron/scintillator sandwich tracking calorimeter For: Little R&D needed, optimised for Golden channel at a high energy NF Against: Relatively high thresholds, no electron ID Liquid argon For: True 3D imaging with pixel size ~ (3mmx3mmx0.3mm) Glasgow/Valencia Glasgow/Valencia Signal efficiency “wrong-sign” muons High granularity dE/dx (PID) Total absorption cal. E E 10E% (e’s) Relatively low energy threshold Charge and scintillation light readout Against: Scale-up issues? Water Cherenkov Liquid scintillator For: For: Excellent e-muon separation Against: Reconstruction: only a low En option (<OGeV) Cherenkov threshold e.g. p K n Size: maybe 1Mton (x20 SuperK) •Very low thresholds possible (200 p.e./MeV) • Well matched to low-energy programme Against: • Reconstruction: similar issues to H2O at high energy, directional information difficult 4 Options Worldwide MIND: x9 MINOS @ NF LAr: single tank (20m drift) vs modular approach (4m maximum drift ) 40m x14m x 14m, B=1T x106 ton-scale water-Cherenkov detectors Memphis in Europe HyperK in Japan LENA: 70kt liquid scintillator (100m x 30m) with active veto for direct cosmics and fast spallation neutrons 5 LAr TPC UK focus has been on a LAr TPC as being the most able to provide a physics program across a broad spectrum of neutrino physics Superb oscillation physics capability to measure oscillations as a function of energy and for n/anti-n separately to break MH/dCP degeneracies in a single experiment (6: 1 mass advantage c.f. Water Cherenkov) Nucleon decay lifetime sensitivities >1034 years: * multi-prong channels: p m - K * kaon channels : p K n (Order -of- magnitude improvement in efficiency for same background over SuperK) Supernova burst neutrinos (for galactic event, expect O10k neutrinos/10secs for 20kt) ; sensitivity to remnant supernova neutrinos (all n-flavours visible) 6 Current State of the Art: ICARUS Jim Strait (Project Director for LBNE):`R&D for an ICARUS-style detector complete – what remains are engineering issues’ 7 LAr: Readout Technology Two main options Single phase e.g. ICARUS Double phase 8 Challenges Towards a Large LAr TPC LAr purity 2-phase charge readout and light readout Drift field DAQ/trigger /electronics Near Detectors Engineering Event reconstruction UK activity (to varying degrees) in all these areas mainly through participation in Euro design studies: EuroNu, IDS-NF, LAGUNA, LAGUNA-LBNO, ASPERA.... 9 UK Focus: Purity/Field Long drift distances in LAr(>10m) demand low electronegative impurities: LAPD@FNAL (30t LAr volume , nonevacuated dewar) recently demonstrated 3ms electron lifetime (100 ppt oxygen equiv.) In right ball-park: 10ms gives 20m attenuation length (for drift of 1 kV/cm) Liverpool /ETHZ tests @CERN demonstrate `piston effect’ and impurity effect on e-lifetime studies (K. Mavrokoridis et al. JINST 6 P08003) HV feed-throughs of ~a few MV can be avoided by internal HV generation (Cockcroft-Walton voltage multiplier) ArDM experiment@CERN has demonstrated 1kV/cm over 1.2m (5m demonstration underway – ARGONTUBE@Bern) 10 UK Focus: Engineering Solutions UK companies* are playing a lead role in defining engineering solutions for a large LAr TPC through LAGUNA-LBNO: Tank design: based on industrial LNG tank with stainless steel or membrane options Non-standard roof : must support field cage inside and electronics from above, feedthroughs etc Delivery of argon underground/ventillation Underground risk assessment Green light for a given project would trigger rapid engineering progress – the UK could be at forefront of this Technodyne * Technodyne International Ltd in collaboration with Alan Auld Ltd, Ryhal Engineering 11 UK Focus: Electronics/DAQ Expertise and experience (LHC, MINOS, T2K,..) Some conceptual design work already starting: Generic DAQ concept for LAr (Proposed by UCL, Manchester for LBNE testbeam) Triggering on events with high background environment e.g. surface LAr detectors at LBNE (Oxford group) Interesting progress in integrating more of the electronics chain (amplifier+digitiser) into dedicated CMOS ASICS running in the liquid volume itself (French and US groups) Real international need for solutions that could put UK in strong position for future involvement 0.35 mm CMOS amp. working at cryogenic temps. (IPNL, Lyon) 12 UK Focus: Reconstruction True automatic event reconstruction only recently seriously developed: Neutrino event topology reconstruction (cellular automaton, principle curves), emag/hadron shower separation (Warwick) First application to ARGONTUBE data – measure diffusion constants over 5m drift (Warwick) nm p m- p LAr simulation ARGONTUBE data Electron/pi0 separation using dE/dx ; energy resolution; hit simulation (QMUL/ETHZ) Cambridge starting to apply particle flow algorithms for LBNE LAr studies Sheffield leading cosmic background studies @ LBNE 13 UK Focus: Readout R&D Liverpool LAr test-stand (40l) working with CEASaclay to investigate bulk MicroMegas for charge amplification Prompt light important for t0/triggering. Liverpool /Sheffield WLS coatings for PMT’s (128nm->430nm). Warwick and Sheffield have investigated possibility of using secondary scintillation emission from TGEM in single phase experiment P K Lightfoot et al., JINST 4:P04002,2009 14 UK Focus:Near Detectors Used to constrain (un-oscillated) event rate at far detector in LBL experiments Essential to control beam flux systematics at 5% or better for dCP-reach in any of the future LBL projects A. Longhin @nuTURN UK experience e.g. T2K ND280 (ECAL, DAQ, engineering) and Glasgow have studied for a Neutrino Factory Hybrid design under consideration: 10- bar argon gas TPC surrounded by scintillator bars (readout as in T2K) to contain showers + 0.5T B-field Near detector concept for LBNO 15 Short-term opportunities (1) MicroBooNE US: MicroBooNE (low E cross sections, MiniBooNE anomaly+R&D) leading onto LBNE 10kt (or even 5kt+5kt) ? Japan: prototype work in 340MeV/c kaon beamline @ JPARC (reconstruction work) leading onto large detector at Okinoshima? 100kt Lar @ Okinoshima AIDA(Euro Integrating Activity Project): Test beam infrastructure (tagged electrons and muons with charge ID) at CERN for neutrino detector prototyping : MiniMIND, DAQ (Glasgow, Liverpool,Oxford, Sheffield) 16 Short term Opportunities (2) LAGUNA-LBNO R&D@CERN A 6x6x6 m3 (300 t) prototype is proposed to be constructed and operated in the CERN North Area To demonstrate feasibility, optimise technologies and evaluate physics performance of the double-phase TPC concept on a large scale Charged particle test beams will be available to collect the first-ever large, controlled, data set to measure calorimetry and PID performance and to validate /develop further our simulation and reconstruction To be positioned in the EHN1 (North Area Hall) - design work already started in GS division for extension of the building Start of construction expected next year Ideal facility for R&D and preparation of the full LAGUNA-LBNO proposal and of interest to other options using LAr e.g. LBNE, Okinoshima. 17 18 Closing Remarks Next project choice clearly still in flux ...... UK focus has been on LAr and groups have managed, with minimal funding, to start laying foundations for contributions to a future project Many areas of R&D are common to all of the detector technology options : e.g. DAQ, underground engineering, near detectors,... Staged solutions involving gradual build-up of detector mass are the favoured strategy (LAGUNA-LBNO, LBNE) Final detector implementations may involve hybrid solutions combining the best from different technologies e.g.: LAGUNA-LBNO far detector GLACIER+LENA installation @ Pyhasalmi to cover high+low E physics programme 19 Thanks to... Kostas Mavrokoridis, Andre Rubbia, Neil Spooner, Lee Thompson, Christos Touramanis,.... 20